论文标题
Cygnus X中的分散$γ$ -Ray排放：对Yan＆Pavaskar的评论
Diffuse $γ$-ray emission in Cygnus X: Comments to Yan & Pavaskar
论文作者
论文摘要
在Arxiv：2211.17057中指出，由于对扩散系数的不正确评估，我们最近的（已发表）论文可能会进行修订，即计算中采用的$ d（e）$。不幸的是，没有迹象表明错误的位置。在这里，我们提供了更具体的机会，通过为社区提供$ d（e）$计算中涉及的方程式的全部描述，{\ tt arxiv}注释中缺少该方程。在这种情况下，我们提到我们的论文中没有使用\ textit {ad hoc}参数化。此外，对注射机制的任何假设在论文中被明确描述为输入因子，显然是模型化程序的一部分，因此最终结果均受到其约束。最后，我们在更广泛的上下文中讨论了扩散系数的计算中，我们认为是关键信息。
It has been pointed out in arXiv:2211.17057 that our recent (published) paper might be revised, due to an incorrect evaluation of the diffusion coefficients, $D(E)$, employed in the calculations. Unfortunately, there is no indication as to where the incorrectness might be. Here we offer the opportunity to be more specific, by providing the community with the whole description of the equations involved in the calculation of $D(E)$, which is missing in the {\tt arXiv} note. In this context, we mention that no \textit{ad hoc} parameterisation has been used in our paper. Furthermore, any assumption on the injection mechanisms is explicitly described in the paper as an input factor and is obviously part of the modelisation procedure, hence the final outcome is subject to it. Finally, we discuss in a more broad context what, in this calculation of the diffusion coefficient, we believe is the key message.
